Spectroscopic survey of IC 1396 identifies 25 new brown dwarfs and measures a star-to-brown-dwarf ratio of 5.0±0.4 that is consistent with other young clusters.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Revealing the substellar population of IC 1396: A spectroscopic survey of brown dwarfs in the region
Spectroscopic survey of IC 1396 identifies 25 new brown dwarfs and measures a star-to-brown-dwarf ratio of 5.0±0.4 that is consistent with other young clusters.